Solving the system of Radiation Magnetohydrodynamics: for solar physical simulations in 3d - Tapa blanda
Sinopsis
We present a Finite-Volume scheme for solving the equations of radiation magnetohydrodynamics. This system is for example used to model the plasma in the solar convection zone and in the solar photosphere. The starting point is a basic scheme for conservation laws. We first study the convergence of the scheme applied to a model problem for the full system of radiation magnetohydrodynamics. We then present modifications of the base scheme which make it possible to approximate the system with an arbitrary equation of state, reduce errors due to a violation of the divergence constraint on the magnetic field, and lead to an improved accuracy in the approximation of solution near an equilibrium state. These modifications are essential for an accurate simulation of processes in the solar atmosphere. For simulations in the solar photosphere, we additionally have to take the radiation intensity into account. A scheme for solving the radiation transport equation is thus a further focus of this study.
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Reseña del editor
We present a Finite-Volume scheme for solving the equations of radiation magnetohydrodynamics. This system is for example used to model the plasma in the solar convection zone and in the solar photosphere. The starting point is a basic scheme for conservation laws. We first study the convergence of the scheme applied to a model problem for the full system of radiation magnetohydrodynamics. We then present modifications of the base scheme which make it possible to approximate the system with an arbitrary equation of state, reduce errors due to a violation of the divergence constraint on the magnetic field, and lead to an improved accuracy in the approximation of solution near an equilibrium state. These modifications are essential for an accurate simulation of processes in the solar atmosphere. For simulations in the solar photosphere, we additionally have to take the radiation intensity into account. A scheme for solving the radiation transport equation is thus a further focus of this study.
Biografía del autor
From 1992 to 1998 Andreas Dedner studied Mathematics at theUniversity of Freiburg. In 1997 he started to develop schemes forsolar physical applications as part of the priority researchprogram ANumE funded by the DFG. The project ended 2003 with thisdissertation, which was awarded the Ferdinant von Lindemann Price.
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Solving the system of Radiation Magnetohydrodynamics
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Südwestdeutscher Verlag Für Hochschulschriften Jul 2009, 2009
ISBN 10: 3838109570
ISBN 13: 9783838109572
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Taschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -We present a Finite-Volume scheme for solving the equations of radiation magnetohydrodynamics. This system is for example used to model the plasma in the solar convection zone and in the solar photosphere. The starting point is a basic scheme for conservation laws. We first study the convergence of the scheme applied to a model problem for the full system of radiation magnetohydrodynamics. We then present modifications of the base scheme which make it possible to approximate the system with an arbitrary equation of state, reduce errors due to a violation of the divergence constraint on the magnetic field, and lead to an improved accuracy in the approximation of solution near an equilibrium state. These modifications are essential for an accurate simulation of processes in the solar atmosphere. For simulations in the solar photosphere, we additionally have to take the radiation intensity into account. A scheme for solving the radiation transport equation is thus a further focus of this study. 352 pp. Englisch. Nº de ref. del artículo: 9783838109572
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Solving the system of Radiation Magnetohydrodynamics
Publicado por
Südwestdeutscher Verlag für Hochschulschriften, 2009
ISBN 10: 3838109570
ISBN 13: 9783838109572
Nuevo
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Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. We present a Finite-Volume scheme for solving the equations of radiation magnetohydrodynamics. This system is for example used to model the plasma in the solar convection zone and in the solar photosphere. The starting point is a basic scheme for conservati. Nº de ref. del artículo: 5405341
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Solving the system of Radiation Magnetohydrodynamics
Publicado por
Südwestdeutscher Verlag Für Hochschulschriften Jul 2009, 2009
ISBN 10: 3838109570
ISBN 13: 9783838109572
Nuevo
Taschenbuch
Librería: buchversandmimpf2000, Emtmannsberg, BAYE, Alemania
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Taschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -We present a Finite-Volume scheme for solving the equations of radiation magnetohydrodynamics. This system is for example used to model the plasma in the solar convection zone and in the solar photosphere. The starting point is a basic scheme for conservation laws. We first study the convergence of the scheme applied to a model problem for the full system of radiation magnetohydrodynamics. We then present modifications of the base scheme which make it possible to approximate the system with an arbitrary equation of state, reduce errors due to a violation of the divergence constraint on the magnetic field, and lead to an improved accuracy in the approximation of solution near an equilibrium state. These modifications are essential for an accurate simulation of processes in the solar atmosphere. For simulations in the solar photosphere, we additionally have to take the radiation intensity into account. A scheme for solving the radiation transport equation is thus a further focus of this study.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 352 pp. Englisch. Nº de ref. del artículo: 9783838109572
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Solving the system of Radiation Magnetohydrodynamics : for solar physical simulations in 3d
Publicado por
Südwestdeutscher Verlag Für Hochschulschriften, 2009
ISBN 10: 3838109570
ISBN 13: 9783838109572
Nuevo
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Librería: AHA-BUCH GmbH, Einbeck, Alemania
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Taschenbuch. Condición: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - We present a Finite-Volume scheme for solving the equations of radiation magnetohydrodynamics. This system is for example used to model the plasma in the solar convection zone and in the solar photosphere. The starting point is a basic scheme for conservation laws. We first study the convergence of the scheme applied to a model problem for the full system of radiation magnetohydrodynamics. We then present modifications of the base scheme which make it possible to approximate the system with an arbitrary equation of state, reduce errors due to a violation of the divergence constraint on the magnetic field, and lead to an improved accuracy in the approximation of solution near an equilibrium state. These modifications are essential for an accurate simulation of processes in the solar atmosphere. For simulations in the solar photosphere, we additionally have to take the radiation intensity into account. A scheme for solving the radiation transport equation is thus a further focus of this study. Nº de ref. del artículo: 9783838109572
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Solving the system of Radiation Magnetohydrodynamics: for solar physical simulations in 3d
Publicado por
Suedwestdeutscher Verlag fuer Hochschulschriften, 2010
ISBN 10: 3838109570
ISBN 13: 9783838109572
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Paperback. Condición: Brand New. 352 pages. 8.66x5.91x0.80 inches. In Stock. Nº de ref. del artículo: 3838109570
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